Baryogenesis in extended inflation. 2: Baryogenesis via primordial black holes

Details Baryogenesis in extended inflation. 2: Baryogenesis via primordial black holes Baryogenesis in extended inflation. 2: Baryogenesis via primordial black holes

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990stin...9026735b&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Asymmetry, Baryons, Black Holes (Astronomy), Collisions, Thermodynamic Equilibrium, Walls, Bubbles, Vacuum

Scientific paper

Baryogenesis at the end of extended inflation is studied. Extended inflation is brought to an end by the collisions of bubble walls surrounding regions of true vacuum, a process which produces particles well out of thermal equilibrium. The possibility that the wall collisions may provide a significant density of primordial black holes is considered and their possible role in generating a baryon asymmetry is examined.

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